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A Michelson-type radio interferometer for university education

  • Jin Koda
  • , James Barrett
  • , Gene Shafto
  • , Jeff Slechta
  • , Tetsuo Hasegawa
  • , Masahiko Hayashi
  • , Stanimir Metchev
  • Stony Brook University
  • National Astronomical Observatory of Japan (NAOJ)
  • Western University

Research output: Contribution to journalArticlepeer-review

8 Scopus citations

Abstract

We report development of a simple and affordable radio interferometer suitable as an educational laboratory experiment. The design of this interferometer is based on the Michelson and Pease stellar optical interferometer, but instead operates at the radio wavelength of ~11 GHz (~2.7 cm), requiring much less stringent optical accuracy in its design and use. We utilize a commercial broadcast satellite dish and feedhorn with two flat side mirrors that slide on a ladder, providing baseline coverage. This interferometer can resolve and measure the diameter of the Sun, even on a day with marginal weather. Commercial broadcast satellites provide convenient point sources for comparison to the Sun's extended disk. The mathematical background of an adding interferometer is presented, as is its design and development, including the receiver system, and sample measurements of the Sun. Results from a student laboratory report are shown. With the increasing importance of interferometry in astronomy, the lack of educational interferometers is an obstacle to training the future generation of astronomers. This interferometer provides the hands-on experience needed to fully understand the basic concepts of interferometry.

Original languageEnglish
Pages (from-to)249-256
Number of pages8
JournalAmerican Journal of Physics
Volume84
Issue number4
DOIs
StatePublished - Apr 1 2016

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